Figure 1 from A Study of a New Increasing Submillimeter Spectral Component of an X28 Solar Flare

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A Study of a New Increasing Submillimeter Spectral Component of an X28 Solar Flare

Authors: A. H. Zhou, J. P. Li, and X. D. Wang

Zhou, Li, & Wang 2011 The Astrophysical Journal 727 42.

Provider: AAS Journals

Caption: Figure 1.

Time profiles of the burst at 405, 212, and 15.6 GHz (top) obtained, respectively, with SST and OVSA in units of thousands of solar flux units. An example of the intense subsecond pulses is shown over a 10 s period during the first peak P1 at the bottom (Kaufmann et al. 2004).

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